Why solar magnetic flux concentrations are bright in molecular bands

Schüssler, M.; Shelyag, S.; Berdyugina, S.; Vögler, A.; Solanki, S. K.

Local TagsRelease HistoryDetailsSummary

Why solar magnetic flux concentrations are bright in molecular bands

Schüssler, M., Shelyag, S., Berdyugina, S., Vögler, A., & Solanki, S. K. (2003). Why solar magnetic flux concentrations are bright in molecular bands. Astrophysical Journal, 597, L173-L176.

Item is Released

show all hide all

Basic

show hide

Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-EE55-0 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-EE56-E

Genre: Journal Article

Files

show Files

Locators

show

Creators

show

hide

Creators:
Schüssler, M.^{1, 2}, Author
Shelyag, S., Author
Berdyugina, S., Author
Vögler, A.², Author
Solanki, S. K.^{1, 2}, Author

Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289

Content

show

hide

Free keywords: -

MPIS_GROUPS: Sun and Heliosphere

Abstract: -

Details

show

hide

Language(s):

Dates: Date issued: 2003

Publication Status: Issued

Pages: -

Publishing info: -

Table of Contents: -

Rev. Type: Peer

Identifiers: BibTex Citekey: Schussler:2003-092

Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show

hide

Title: Astrophysical Journal

Source Genre: Journal

Creator(s):

Affiliations:

Publ. Info: -

Pages: - Volume / Issue: 597 Sequence Number: - Start / End Page: L173 - L176 Identifier: -